SDO HMI 2011-10-25 15:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.22 | 168.70 | 26.48 | 137.06 | -21.69 | 331.28 | 46.05 | 237.56 | 0.7948 | -382.1 | -325.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.47 | 0.00 | 3.13 | -18.94 | 337.35 | 52.12 | 243.38 | 0.8372 | 559.0 | 528.6 | |
| 0.00 | 1.65 | 0.00 | 1.45 | -17.81 | 336.81 | 51.58 | 244.46 | 0.8290 | 666.0 | 502.7 | |
| 4.17 | 4.69 | 3.72 | 4.18 | -19.07 | 336.89 | 51.66 | 243.06 | 0.8338 | 649.4 | 568.8 | |
| 0.96 | 1.39 | 0.85 | 1.24 | -19.58 | 336.76 | 51.53 | 242.43 | 0.8343 | 448.9 | 410.8 | |
| 0.00 | 1.39 | 0.00 | 1.22 | -19.09 | 336.24 | 51.01 | 242.78 | 0.8282 | 455.0 | 358.8 | |
| 1.74 | 3.56 | 1.52 | 3.11 | -19.07 | 335.98 | 50.75 | 242.69 | 0.8259 | 678.0 | 637.0 | |
| 0.00 | 0.96 | 0.00 | 0.83 | -19.30 | 335.63 | 50.40 | 242.29 | 0.8236 | 558.0 | 494.5 | |
| 0.00 | 0.69 | 0.00 | 0.61 | -20.96 | 335.57 | 50.34 | 240.39 | 0.8291 | 348.0 | 312.6 | |
| 0.00 | 1.74 | 0.00 | 1.42 | -21.74 | 331.61 | 46.38 | 237.69 | 0.7978 | -438.0 | -254.9 | |
| 5.30 | 19.97 | 4.27 | 16.10 | -21.34 | 331.07 | 45.84 | 237.88 | 0.7912 | -736.7 | -280.7 | |
| 1.82 | 126.59 | 1.47 | 101.68 | -21.76 | 330.97 | 45.74 | 237.35 | 0.7922 | -531.0 | -421.0 | |
| 0.00 | 1.30 | 0.00 | 1.05 | -21.49 | 330.86 | 45.62 | 237.60 | 0.7899 | -743.0 | -690.9 | |
| 0.00 | 1.30 | 0.00 | 1.04 | -20.95 | 330.59 | 45.36 | 238.10 | 0.7851 | -432.0 | -414.5 | |
| 18.23 | -11.00 | 14.65 | -11.00 | -22.20 | 330.45 | 45.22 | 236.59 | 0.7896 | -959.1 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |